New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models
- 31 December 1997
- Vol. 130 (2) , 534-539
- https://doi.org/10.1006/icar.1997.5812
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This publication has 24 references indexed in Scilit:
- Solar models with helium and heavy-element diffusionReviews of Modern Physics, 1995
- Condensation of Methane, Ammonia, and Water and the Inhibition of Convection in Giant PlanetsScience, 1995
- Nonadiabatic Models of Jupiter and SaturnIcarus, 1994
- Are the Giant Planets Fully Convective?Icarus, 1994
- The molecular-metallic transition of hydrogen and the structure of Jupiter and SaturnThe Astrophysical Journal, 1992
- The abundance and distribution of water vapor in the Jovian troposphere as inferred from Voyager IRIS observationsThe Astrophysical Journal, 1992
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- The helium abundance of Saturn from Voyager measurementsThe Astrophysical Journal, 1984
- Effects of differential rotation on the gravitational figures of Jupiter and SaturnIcarus, 1982
- The C/H ratio in Jupiter from the Voyager infrared investigationThe Astrophysical Journal, 1982